Despicable Dark Relics: generated by gravity with unconstrained masses
Malcolm Fairbairn, Kimmo Kainulainen, Tommi Markkanen, Sami Nurmi

TL;DR
This paper introduces a gravitational mechanism during reheating that can produce a wide range of dark relics with masses from keV to 10^8 GeV, which are undetectable by current non-gravitational searches.
Contribution
It demonstrates a generic, efficient gravitational process for dark relic production during reheating, applicable for any inert scalar with non-minimal curvature coupling.
Findings
Relic abundance can match observed dark matter for various masses.
Production mechanism is efficient for natural coupling values around unity.
Relics are undetectable by current non-gravitational searches.
Abstract
We demonstrate the existence of a generic, efficient and purely gravitational channel producing a significant abundance of dark relics during reheating after the end of inflation. The mechanism is present for any inert scalar with the non-minimal curvature coupling and the relic production is efficient for natural values . The observed dark matter abundance can be reached for a broad range of relic masses extending from to , depending on the scale of inflation and the dark sector couplings. Frustratingly, such relics escape direct, indirect and collider searches since no non-gravitational couplings to visible matter are needed.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
